SDO HMI 2011-06-05 22:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 35.55 | 179.00 | 19.14 | 96.52 | 9.11 | 336.73 | -21.36 | 65.97 | 0.3955 | -747.9 | -342.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.90 | 0.00 | 1.00 | 7.46 | 339.25 | -18.84 | 67.59 | 0.3478 | -793.0 | -472.3 | |
| 2.17 | 135.76 | 1.17 | 73.09 | 9.19 | 337.36 | -20.73 | 65.16 | 0.3867 | -1355.6 | -439.4 | |
| 25.24 | -2.00 | 13.59 | -2.00 | 9.28 | 336.96 | -21.13 | 65.34 | 0.3931 | -1239.9 | 999999 | |
| 1.54 | 8.77 | 0.83 | 4.71 | 8.17 | 336.96 | -21.13 | 67.99 | 0.3865 | -743.6 | 305.1 | |
| 0.00 | 1.36 | 0.00 | 0.73 | 8.26 | 336.69 | -21.40 | 68.01 | 0.3911 | -733.0 | -546.7 | |
| 0.00 | 2.35 | 0.00 | 1.27 | 8.57 | 336.48 | -21.62 | 67.46 | 0.3961 | -767.0 | -707.0 | |
| 4.70 | 21.35 | 2.53 | 11.50 | 8.11 | 336.37 | -21.72 | 68.65 | 0.3950 | -769.0 | -95.6 | |
| 0.00 | 1.09 | 0.00 | 0.59 | 11.10 | 336.00 | -22.09 | 62.19 | 0.4190 | -699.0 | -504.0 | |
| 1.90 | -7.00 | 1.02 | -7.00 | 7.62 | 336.13 | -21.96 | 70.03 | 0.3960 | 880.6 | 999999 | |
| 0.00 | 1.90 | 0.00 | 1.03 | 8.02 | 335.91 | -22.18 | 69.25 | 0.4014 | -758.0 | -615.2 | |
| 0.00 | 0.90 | 0.00 | 0.51 | 12.88 | 331.84 | -26.26 | 62.45 | 0.4884 | 821.0 | 571.1 | |
| 0.00 | 1.18 | 0.00 | 0.67 | 11.11 | 331.33 | -26.76 | 66.22 | 0.4848 | 669.0 | 566.2 | |
| 0.00 | 0.90 | 0.00 | 0.52 | 12.60 | 330.64 | -27.45 | 63.92 | 0.5028 | 818.0 | 707.9 | |
| 0.00 | 1.54 | 0.00 | 0.90 | 12.98 | 328.82 | -29.27 | 64.56 | 0.5296 | 496.0 | 387.1 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |